activity
20232026
most citedNew and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects

58 citations · 118 across the 17 of their papers we have counts for

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Showing 2024Show all

6 papers · 1 filter

gr-qc2024★ 11 cited

On the Role of Muons in Binary Neutron Star Mergers: First Simulations

Henrique Gieg, Federico Schianchi, Maximiliano Ujevic +1

In this work we present a set of binary neutron star (BNS) merger simulations including the net muon fraction as an additional degree-of-freedom in the equation of state (EoS) and…

astro-ph.HE2024★ 15 cited

The impact of dark matter on tidal signatures in neutron star mergers with Einstein Telescope

Hauke Koehn, Edoardo Giangrandi, Nina Kunert +3

If dark matter (DM) accumulates inside neutron stars (NS), it changes their internal structure and causes a shift of the tidal deformability from the value predicted by the dense-m…

gr-qc2024

General Relativistic Magneto-Hydrodynamic Simulations with BAM: Implementation and Code Comparison

Anna Neuweiler, Tim Dietrich, Bernd Brügmann +7

Binary neutron star mergers are among the most energetic events in our Universe, with magnetic fields significantly impacting their dynamics, particularly after the merger. While n…

astro-ph.HE2024★ 19 cited

Using Equation of State Constraints to Classify Low-Mass Compact Binary Mergers

Jacob Golomb, Isaac Legred, Katerina Chatziioannou +2

Compact objects observed via gravitational waves are classified as black holes or neutron stars primarily based on their inferred mass with respect to stellar evolution expectation…

astro-ph.HE2024

Black-hole formation in binary neutron star mergers: The impact of spin on the prompt-collapse scenario

Federico Schianchi, Maximiliano Ujevic, Anna Neuweiler +3

Accurate modeling of the multi-messenger signatures connected to binary neutron star mergers requires proper knowledge on the final remnant's fate and the conditions under which bl…

astro-ph.HE2024★ 9 cited

From existing and new nuclear and astrophysical constraints to stringent limits on the equation of state of neutron-rich dense matter

Hauke Koehn, Henrik Rose, Peter T. H. Pang +10

Through continuous progress in nuclear theory and experiment and an increasing number of neutron-star observations, a multitude of information about the equation of state (EOS) for…